γ-ray observations of extraterrestrial neutrino track event positions

الأصل · EN

In this paper we report the results of a γ-ray study of IceCube's extraterrestrial neutrino candidates detected as track-like events. Using 70 months of Fermi-LAT observations, a likelihood analysis of all 1-300 GeV photons within 5 degrees of the track-like neutrino candidates' origin was undertaken, to search for spatially coincident γ-ray emission. One of IceCube's HESE track events was found to be spatially coincident with a γ-ray bright active galactic nucleus (AGN), PKS 0723-008. We find however, that the chance probability for Fermi-LAT detected AGN to be spatially coincident with a single HESE track-like event is high (37%). We therefore find no evidence of γ-ray emission associated with the detection of IceCube's HESE track-like neutrino candidates. Upper limits were calculated in the energy range of 1-300 GeV, assuming a point source origin for the neutrino events considered. The implications for the non-detection of γ-ray emission from the source of the HESE track-like events are briefly discussed. The large time period analysed in our study did however, reveal two new γ-ray point sources. With a flux of (1.28 ± 0.08) × 10⁻⁹ photons cm⁻² s⁻¹, in the 1-300 GeV energy range, and an associated TS value of 220.6, one of these new point sources is positionally coincident with the AGN PKS 1346-112. The other point source has a 1-300 GeV flux of (7.95 ± 1.23) × 10⁻¹⁰ photons cm⁻² s⁻¹ and an associated TS value of 92.4. This new point source is spatially coincident with the radio source NVSS J072534+021645 suggesting that it too is an AGN.